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Skin-Effect Description in Electromagnetism with a Scaled Asymptotic Expansion
Victor Péron, Gabriel Caloz, Monique Dauge
To cite this version:
Victor Péron, Gabriel Caloz, Monique Dauge. Skin-Effect Description in Electromagnetism with a Scaled Asymptotic Expansion. WAVES 2009 The 9th International Conference on Mathematical and Numerical Aspects of Waves Propagation, Jun 2009, Pau, France. �inria-00528514�
Skin-Effect Description in Electromagnetism with a Scaled Asymptotic Expansion V. P´eron1,∗, G. Caloz1, M. Dauge1
1 Numerical Analysis, IRMAR, University of Rennes 1, Rennes, France
∗Email: victor.peron@univ-rennes1.fr Abstract
We study a transmission problem in high contrast media. The 3-D case of the Maxwell equations in harmonic regime is considered. We derive an asymp- totic expansion with respect to a small parameter δ >0 related to high conductivity. This expansion is theoretically justified at any order. Numerical sim- ulations highlight the skin-effect and the expansion accuracy.
Introduction
We consider the diffraction problem of waves by highly conducting materials in electromagnetism.
The high conductivity reduces the penetration of the wave to a boundary layer, see [1]. The physical model is the following. Ωcd is an open bounded domain in R3 with connected complement, occupied by a con- ducting medium. Ωcd is embedded in an insulating medium Ωis. We suppose that their common inter- face Σ is smooth. We define Ω = Ωcd ∪Σ∪Ωis. We denote by δ a small parameter which is inversely proportional to the square root of the conductivity σ. The depth of the boundary layer is proportional to δ. We first give the formal construction of the asymptotic expansion. Then, we prove optimal error estimates. Finally, we present numerical simulations in axisymmetric geometry.
1 Scaled asymptotic expansion
Eliminating the magnetic field Hδ from Maxwell equations, we perform a study in electric fieldEδ. 1.1 Normal coordinates
To describe the boundary layer in Ωcd, we define a local normal coordinate system (yα, y3), α∈ {1,2}, in a tubular neighborhood O of Σ, y3 ∈(0, h0). The euclidian metric inOis denoted by (gij)i,j∈{1,2,3}. We adopt the tensorial calculus, see [2], to write Maxwell equations in these coordinates. The curl operator writes
( (curlE)α = √1g3βα(∂3Eβ−∂βE3) (curlE)3 = √1g3αβDαhEβ
with g = det(gij), ijk the Levi-Civita symbol, and Dh a covariant derivative defined for h=y3, see [2].
1.2 Scaling and ansatz
We perform the scaling Y3= yδ3 inO, and expand the 3D Maxwell operator in power of series ofδ. This leads to postulate the following expansions
Eisδ(x)∼X
j≥0
Eisj(x)δj, Ecdδ (x)∼X
j≥0
Ecdj (x;δ)δj (1)
respectively in Ωis, and Ωcd, with Ecdj (x;δ) = Wcdj (yα, yδ3) when (yα, y3) ∈ O. We prove that Wcd0 = 0, and Wcdj (., Y3) = exp(−λY3)[a0 +.. + aj−1Y3j−1], with <(λ) > 0. According to Faraday’s law Hδ = 1/(iκµ0) curlEδ, κ > 0 (a wave number), we derive the expansion of the magnetic field.
2 Uniform a priori estimate
A regularized variational formulation of our prob- lem in the domain Ω using the space XN(δ) = {E ∈ H(curl,Ω)| ε(δ)E ∈ H(div,Ω), E × n = 0 on ∂Ω} is:
Find Eδ ∈XN(δ) such that for all u∈XN(δ) Z
Ω
curlE·curlu+divε(δ)Edivε(δ)u−κ2ε(δ)E·udx
= Z
Ω
(Fδ·u− 1
κ2 divFδdivε(δ)u)dx, (2) with ε(δ) = µ1
0(1Ωis + (1 +δi2)1Ωcd), µ0 > 0, and Fδ ∈ H(div,Ω). Under a spectral hypothesis on κ, we prove that∃δ0 >0 small enough such that ∀δ ∈ (0, δ0), (2) has a unique solution Eδ ∈ XN(δ), and there is a constantC >0 independent ofδ such that
kcurlEδk0,Ω+kdivε(δ)Eδk0,Ω+kEδk0,Ω
+1
δkEδk0,Ωcd ≤CkFδkH(div,Ω). We prove this estimate using a technique of vector potential, see [3]. Defining Rδm from (1) by remov- ing to Eδ them+ 1 first-terms of the expansion, we deduce optimal error estimates for the truncated ex- pansions
kRδmkH(curl,Ω)+kdivε(δ)Rδmk0,Ω+1
δkRδmk0,Ωcd ≤Cδm−1.
3 Numerical simulations
Here we present numerical experiments to illus- trate the accuracy of the asymptotic expansion. We perform our analysis to the magnetic field and re- strict ourselves to axisymmetric domains with an or- thoradial data. After having meshed the domain, we compute the orthoradial component of the mag- netic field Hθ with the finite element library Melina, see [4]. The numerical method uses a variational form with unknown Hθ(r, z) in a meridian domain, which is meshed in such a way the boundary layer is correctly taken into account, see Figure 1 for spheroidal domains. We extract values of |Hθ(y3)|
Figure 1: |=Hθ| forσ= 5S.m−1 and 80S.m−1
along edges of the mesh for z = 0. We perform a linear regression from values of log10|Hθ(y3)| in a depth-skin defined by skin(σ) = √
2δ(σ)/κ, cor- responding to n(σ) points on the mesh, see Fig- ure 2 for spherical domains with y3 = 2−r. We
0 0.5 1 1.5 2
−6
−5
−4
−3
−2
−1 0 1 2
2 − r
Figure 2: log10|Hθ(2−r)| forσ= 5S.m−1
get a ”numerical” slope s(σ). Let Hcdθ,1 be the or- thoradial component of Hcd0 (x;δ) + δHcd1 (x;δ) (the truncated asymptotic expansion of Hδ). We prove that log10|Hθ,1cd(y3)|=α(σ)y3+ log10|Hθ,0is
|Σ|+O(δ).
α(σ) = β−1/skin(σ)
/ln 10 is a ”theoretical” slope, andβ depends on the curvature on Σ. The accuracy of the expansion is tested by representing the relative error between ”numerical” and ”theoretical” slopes:
error(σ) =|α(σ)−s(σ)|
|α(σ)|, see Figure 3.
σ (S.m−1) 5 20 80
skin(σ) (cm) 10.3 5.15 2.58
n(σ) 7 5 3
s(σ) −3,65542 −7,88390 −16,27916 α(σ) −3,67331 −7,88950 −16,32188 error(σ) (%) 0,48 0,07 0,26
Figure 3: Relative error in spheroidal domains
References
[1] H. Haddar, P. Joly, H.N. Nguyen, Construction and analysis of approximate models for electro- magnetic scattering from imperfectly conducting scatterers, Math. Models Methods Appl. Sci., vol. 18, 10, 1787-1827, 2008.
[2] E. Faou,Elasticity on a thin shell: Formal series solution, Asymptotic Analysis,31(3-4):317-361, 2002.
[3] C. Amrouche, C. Bernardi, M. Dauge, V.Girault, Vector Potentials in Three- dimensional Non-smooth Domains, Math.
Meth. Appl. Sci., 21, 823-864, 1998.
[4] D. Martin, Melina. http://anum-maths.univ- rennes1.fr/melina/